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is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2406.11937">arXiv:2406.11937</a> <span> [<a href="https://arxiv.org/pdf/2406.11937">pdf</a>, <a href="https://arxiv.org/format/2406.11937">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/19/11/P11025">10.1088/1748-0221/19/11/P11025 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Using graph neural networks to reconstruct charged pion showers in the CMS High Granularity Calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Aamir%2C+M">M. Aamir</a>, <a href="/search/physics?searchtype=author&query=Adamov%2C+G">G. Adamov</a>, <a href="/search/physics?searchtype=author&query=Adams%2C+T">T. Adams</a>, <a href="/search/physics?searchtype=author&query=Adloff%2C+C">C. Adloff</a>, <a href="/search/physics?searchtype=author&query=Afanasiev%2C+S">S. Afanasiev</a>, <a href="/search/physics?searchtype=author&query=Agrawal%2C+C">C. Agrawal</a>, <a href="/search/physics?searchtype=author&query=Agrawal%2C+C">C. Agrawal</a>, <a href="/search/physics?searchtype=author&query=Ahmad%2C+A">A. Ahmad</a>, <a href="/search/physics?searchtype=author&query=Ahmed%2C+H+A">H. A. Ahmed</a>, <a href="/search/physics?searchtype=author&query=Akbar%2C+S">S. Akbar</a>, <a href="/search/physics?searchtype=author&query=Akchurin%2C+N">N. Akchurin</a>, <a href="/search/physics?searchtype=author&query=Akgul%2C+B">B. Akgul</a>, <a href="/search/physics?searchtype=author&query=Akgun%2C+B">B. Akgun</a>, <a href="/search/physics?searchtype=author&query=Akpinar%2C+R+O">R. O. Akpinar</a>, <a href="/search/physics?searchtype=author&query=Aktas%2C+E">E. Aktas</a>, <a href="/search/physics?searchtype=author&query=Kadhim%2C+A+A">A. Al Kadhim</a>, <a href="/search/physics?searchtype=author&query=Alexakhin%2C+V">V. Alexakhin</a>, <a href="/search/physics?searchtype=author&query=Alimena%2C+J">J. Alimena</a>, <a href="/search/physics?searchtype=author&query=Alison%2C+J">J. Alison</a>, <a href="/search/physics?searchtype=author&query=Alpana%2C+A">A. Alpana</a>, <a href="/search/physics?searchtype=author&query=Alshehri%2C+W">W. Alshehri</a>, <a href="/search/physics?searchtype=author&query=Dominguez%2C+P+A">P. Alvarez Dominguez</a>, <a href="/search/physics?searchtype=author&query=Alyari%2C+M">M. Alyari</a>, <a href="/search/physics?searchtype=author&query=Amendola%2C+C">C. Amendola</a>, <a href="/search/physics?searchtype=author&query=Amir%2C+R+B">R. B. Amir</a> , et al. (550 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2406.11937v3-abstract-short" style="display: inline;"> A novel method to reconstruct the energy of hadronic showers in the CMS High Granularity Calorimeter (HGCAL) is presented. The HGCAL is a sampling calorimeter with very fine transverse and longitudinal granularity. The active media are silicon sensors and scintillator tiles readout by SiPMs and the absorbers are a combination of lead and Cu/CuW in the electromagnetic section, and steel in the hadr… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2406.11937v3-abstract-full').style.display = 'inline'; document.getElementById('2406.11937v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2406.11937v3-abstract-full" style="display: none;"> A novel method to reconstruct the energy of hadronic showers in the CMS High Granularity Calorimeter (HGCAL) is presented. The HGCAL is a sampling calorimeter with very fine transverse and longitudinal granularity. The active media are silicon sensors and scintillator tiles readout by SiPMs and the absorbers are a combination of lead and Cu/CuW in the electromagnetic section, and steel in the hadronic section. The shower reconstruction method is based on graph neural networks and it makes use of a dynamic reduction network architecture. It is shown that the algorithm is able to capture and mitigate the main effects that normally hinder the reconstruction of hadronic showers using classical reconstruction methods, by compensating for fluctuations in the multiplicity, energy, and spatial distributions of the shower's constituents. The performance of the algorithm is evaluated using test beam data collected in 2018 prototype of the CMS HGCAL accompanied by a section of the CALICE AHCAL prototype. The capability of the method to mitigate the impact of energy leakage from the calorimeter is also demonstrated. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2406.11937v3-abstract-full').style.display = 'none'; document.getElementById('2406.11937v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 17 June, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 19 (2024) P11025 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2309.05481">arXiv:2309.05481</a> <span> [<a href="https://arxiv.org/pdf/2309.05481">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Materials Science">cond-mat.mtrl-sci</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Applied Physics">physics.app-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Chemical Physics">physics.chem-ph</span> </div> </div> <p class="title is-5 mathjax"> Photovoltaic potential of tin perovskites revealed through layer-by-layer investigation of optoelectronic and charge transport properties </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Aldamasy%2C+M+H">Mahmoud H. Aldamasy</a>, <a href="/search/physics?searchtype=author&query=Musiienko%2C+A">Artem Musiienko</a>, <a href="/search/physics?searchtype=author&query=Rusu%2C+M">Marin Rusu</a>, <a href="/search/physics?searchtype=author&query=Regaldo%2C+D">Davide Regaldo</a>, <a href="/search/physics?searchtype=author&query=Zho%2C+S">Shengnan Zho</a>, <a href="/search/physics?searchtype=author&query=Hampel%2C+H">Hannes Hampel</a>, <a href="/search/physics?searchtype=author&query=Frasca%2C+C">Chiara Frasca</a>, <a href="/search/physics?searchtype=author&query=Iqbal%2C+Z">Zafar Iqbal</a>, <a href="/search/physics?searchtype=author&query=Gries%2C+T+W">Thomas W. Gries</a>, <a href="/search/physics?searchtype=author&query=Li%2C+G">Guixiang Li</a>, <a href="/search/physics?searchtype=author&query=Aktas%2C+E">Ece Aktas</a>, <a href="/search/physics?searchtype=author&query=Nasti%2C+G">Giuseppe Nasti</a>, <a href="/search/physics?searchtype=author&query=Li%2C+M">Meng Li</a>, <a href="/search/physics?searchtype=author&query=Pascual%2C+J">Jorge Pascual</a>, <a href="/search/physics?searchtype=author&query=Hartono%2C+N+T+P">Noor Titan Putri Hartono</a>, <a href="/search/physics?searchtype=author&query=Wang%2C+Q">Qiong Wang</a>, <a href="/search/physics?searchtype=author&query=Unold%2C+T">Thomas Unold</a>, <a href="/search/physics?searchtype=author&query=Abate%2C+A">Antonio Abate</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2309.05481v3-abstract-short" style="display: inline;"> Tin perovskites are the most promising environmentally friendly alternative to lead perovskites. Among tin perovskites, FASnI3 (CH4N2SnI3) shows optimum band gap, and easy processability. However, the performance of FASnI3 based solar cells is incomparable to lead perovskites for several reasons, including energy band mismatch between the perovskite absorber film and the charge transporting layers… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2309.05481v3-abstract-full').style.display = 'inline'; document.getElementById('2309.05481v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2309.05481v3-abstract-full" style="display: none;"> Tin perovskites are the most promising environmentally friendly alternative to lead perovskites. Among tin perovskites, FASnI3 (CH4N2SnI3) shows optimum band gap, and easy processability. However, the performance of FASnI3 based solar cells is incomparable to lead perovskites for several reasons, including energy band mismatch between the perovskite absorber film and the charge transporting layers (CTLs) for both types of carriers, i.e., for electrons (ETLs) and holes (HTLs). However, the band diagrams in the literature are inconsistent, and the charge extraction dynamics are poorly understood. In this paper, we study the energy band positions of FASnI3 based perovskites using Kelvin probe (KP) and photoelectron yield spectroscopy (PYS) to provide a precise band diagram of the most used device stack. In addition, we analyze the defects within the current energetic landscape of tin perovskites. We uncover the role of bathocuproine (BCP) in enhancing the electron extraction at the fullerene C60/BCP interface. Furthermore, we used transient surface photovoltage (tr-SPV) for the first time for tin perovskites to understand the charge extraction dynamics of the most reported HTLs such as NiOx and PEDOT, and ETLs such as C60, ICBA, and PCBM. Finally, we used Hall effect, KP, and time-resolved photoluminescence (TRPL) to estimate an accurate value of the p-doping concentration in FASnI3 and showed a consistent result of 1.5 * 1017 cm-3. Our findings prove that the energetic system of tin halide perovskites is deformed and should be redesigned independently from lead perovskites to unlock the full potential of tin perovskites. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2309.05481v3-abstract-full').style.display = 'none'; document.getElementById('2309.05481v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 October, 2023; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 11 September, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2023. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">22 pages, 5 figures</span> </p> </li> </ol> <div class="is-hidden-tablet">  <span class="help" 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